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<ri:Resource created="2015-10-23T07:38:33Z" status="active" updated="2026-03-17T20:07:16Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Metal-poor stars speckle interferometry</title><shortName>J/other/AstBu/63</shortName><identifier>ivo://CDS.VizieR/J/other/AstBu/63.278</identifier><altIdentifier>doi:10.26093/cds/vizier/dv/gdkchi</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rastegaev D.A.</name></creator><creator><name>Balega Yu.Yu.</name></creator><creator><name>Maksimov A.F.</name></creator><creator><name>Malogolovets E.V.,Dyachenko V.V.</name></creator><date role="Updated">2026-03-17T20:07:16Z</date><date role="Created">2015-10-23T07:38:33Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>multiple-stars</subject><description>The results of speckle interferometric observations of 115 metal-poor stars ([m/H]&lt;-1) within 250pc from the Sun and with proper motions mu&gt;~0.2"/yr, made with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences, are reported. Close companions with separations ranging from 0.034" to 1" were observed for 12 objects - G76-21, G59-1, G63-46, G135-16, G168-42, G141-47, G142-44, G190-10, G28-43, G217-8, G130-7, and G89-14 - eight of them are astrometrically resolved for the first time. The newly resolved systems include one triple star - G190-10. 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